IRAS 04509-6922
red Supergiant in the Large Magellanic cloud
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IRAS 04509-6922 is an AGB in the Large Magellanic Cloud.
IRAS 04509-6922’s minimum radius is 1,027 solar radii (1,430,286,468 km) (1,430,286,468,000 m).[1]
IRAS 04509-6922’s maximum radius is 2,249 solar radii (3,132,146,316 km) (3,132,146,316,000 m), but this is unlikely.[1]
Another estimate suggests a radius of 1,187 solar radii.[2]
It has a spectral type of M10.
References
change- ↑ 1.0 1.1 Goldman, Steven R.; van Loon, Jacco Th.; Zijlstra, Albert A.; Green, James A.; Wood, Peter R.; Nanni, Ambra; Imai, Hiroshi; Whitelock, Patricia A.; Matsuura, Mikako; Groenewegen, Martin A. T.; Gómez, José F. (2017-02-11). "The wind speeds, dust content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity". Monthly Notices of the Royal Astronomical Society. 465 (1): 403–433. doi:10.1093/mnras/stw2708. ISSN 0035-8711.
{{cite journal}}: CS1 maint: unflagged free DOI (link) - ↑ Groenewegen, M. A. T.; Sloan, G. C. (2018-01). "Luminosities and mass-loss rates of Local Group AGB stars and red supergiants". Astronomy & Astrophysics. 609: A114. doi:10.1051/0004-6361/201731089. ISSN 0004-6361.
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